ethan fukuda cody tamura period 1

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Supernova Ethan Fukuda Cody Tamura Period 1

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What is a supernova? An exploding star reaching the end of its life They emit more energy than the sun will in its lifetime The blast is so bright, it will often outshine a galaxy for up to a couple of months

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Page 1: Ethan Fukuda Cody Tamura Period 1

SupernovaEthan FukudaCody Tamura

Period 1

Page 2: Ethan Fukuda Cody Tamura Period 1

What is a supernova?

An exploding star reaching the end of its life

They emit more energy than the sun will in its lifetime

The blast is so bright, it will often outshine a galaxy for up to a couple of months

Page 3: Ethan Fukuda Cody Tamura Period 1

What is a supernova?

On average, one will occur every 50 years in a galaxy

In the universe, a star explodes every other second (that’s a lot)

Page 4: Ethan Fukuda Cody Tamura Period 1

The SunThe Sun does not have enough mass to turn into a supernova

However, when it runs out of its nuclear fuel, it will turn into a red giant and vaporize anything in its path

Then it will cool to a white dwarf

Page 5: Ethan Fukuda Cody Tamura Period 1

Types of supernovae

Type I – a star gathers matter from a neighbor star until a nuclear reaction occurs

Type II – a star runs out of nuclear fuel and implodes under its own gravity

Page 6: Ethan Fukuda Cody Tamura Period 1

Type ILack a hydrogen signature in their spectrum of light

Believed to originate from white dwarves

Neighbor stars give off gas that collapses the white dwarf and a nuclear reaction occurs

Page 7: Ethan Fukuda Cody Tamura Period 1

Type I continuedThey lack hydrogen compared to other types of supernovas

They are brighter than type II supernovas

A white dwarf can only support a mass of 1.38 Solar masses, and if it goes above, it will start to collapse than explode

Another way is if a white dwarf combines with another star, which is a very rare event

Page 8: Ethan Fukuda Cody Tamura Period 1

Type IIMust be several times larger than the Sun

At its death, a star will stratify the elements within itself

They begin to implode

The implosion bounces off the core and creates an explosion

Page 9: Ethan Fukuda Cody Tamura Period 1

Type II continuedBecause of this implosion, type II supernovas are known as core-collapse supernovas

The difference between a type ll supernova and the other types of supernovas, is that hydrogen is present in its spectrum

A type ll supernova is a massive star, which generates energy by nuclear fusion of elements

Page 10: Ethan Fukuda Cody Tamura Period 1

The Brightest Supernova

It was seen September 2006, ground based telescopes and from NASA’s Chandra X-ray observatory.

This was the biggest and brightest stellar blast ever recorded, and could be a newly discovered type of supernova.

Scientists estimate that the explosion is equal to that of an explosion of a star with 150 times more mass than our sun.